Eccentric & Mean Anomaly: Difference & Drawing

AI Thread Summary
The discussion clarifies the differences between Eccentric Anomaly and Mean Anomaly in orbital mechanics. Eccentric Anomaly is represented by the angle E in relation to an ellipse, while Mean Anomaly is a mathematical average that ensures a constant rate of increase, despite the variable speed of a planet in its orbit. The Mean Anomaly is derived from the Eccentric Anomaly by averaging it over the entire orbit, similar to the concept of a Mean Solar Day. The drawing illustrates the relationship between these anomalies, but the Mean Anomaly cannot be visually represented in the same way. Understanding these distinctions is crucial for accurately modeling celestial orbits.
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What is the difference between the drawing of the Eccentric Anomaly and the Mean Anomaly.
http://www.philosophaie.com/EA.png
One has a circle radius "a" inscribed an ellipse with a focus "F". The True Anomaly makes "f" makes an angle to point "P" then a perpendicular is drawn to a point on the circle where a line is drawn to the center.

What is this angle Mean or Eccentric? How do you draw the other Anomaly?
 
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Is Mean Anomaly from point "P" on the ellipse to the center?
 
The mean anomaly is a mathematical construct. Neither the True anomaly (f in the drawing) nor the Eccentric anomaly (E in the drawing) change at a constant rate, because the planet goes more slowly when it is far away from the Sun than when it is close to the sun. So the Mean Anomaly is obtained by taking E and averaging it over the whole orbit so that M is always increasing at a constant rate. It is similar in concept to the "Mean Solar Day", where we take the average length of the day over the whole year and create a day that is always the same length, even though the actual length of the day changes slightly as we go through the year. Since it is a construct, I don't know of a way to picture it on the drawing.
 
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